Hot HB stars in globular clusters - Physical parameters and consequences for theory: VI. The second parameter pair M 3 and M 13

Astronomy and Astrophysics

Volumn 405, Issue 1, 2003, Pages 135-148

  Moehler, S ^a,b   Landsman, W B ^c   Sweigart, A V ^c   Grundahl, F ^d  

^a UNIVERSITY OF KIEL   (Germany)

^b UNIVERSITY OF ERLANGEN NUREMBERG   (Germany)

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

^d AARHUS UNIVERSITY   (Denmark)

Author keywords

Galaxy: globular clusters: individual: M 13; Galaxy: globular clusters: individual: M 3; Stars: atmospheres; Stars: evolution; Stars: horizontal branch

Indexed keywords

DIFFUSION; INFRARED IMAGING; PHOTOMETRY; SOLAR RADIATION; UPPER ATMOSPHERE;

GLOBULAR CLUSTERS;

GALAXIES;

EID: 0038756490     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030622     Document Type: Article

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